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REDUCE_FLAT
- Reduces an imaging flat field
- Description:
- This reduces a flat field in the conventional manner consisting of
bad-pixel masking, dark subtraction, and normalisation by the
mean of the image. It also files the normalised flat-field frame
for use by subsequent flat-fielding operations.
- Notes:
- This recipe will reduce any image passed to it. Care must
be taken to ensure that a proper flat-field image will be reduced.
- The bad pixel mask applied is $ORAC_DATA_CAL/bpm.
- The flat field is normalised using a clipped mean, where
the clipping levels are 2, 3, and 3 standard deviationss. This
value is effectively the mode of the image. The entire image is
divided by this value to normalise it.
- Intermediate frames are deleted.
-
Output Data
:
- The flat is called flat_<frame_number>.
- The flat is filed in $ORAC_DATA_OUT/index.flat.
- Implementation Status:
- The processing engines are from the Starlink packages
KAPPA and CCDPACK.
- Uses the Starlink NDF format.
- History is recorded within the data files.
- The title of the data is propagated through the intermediate file
to the flat.
- Variance information is not supported.
Next: SKY_AND_JITTER - Reduces a ``combined jitter'' photometry observation
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Previous: REDUCE_DARK - Averages and files observations as the current dark
ORAC-DR -- imaging data reduction
Starlink User Note 232
Malcolm J. Currie
Brad Cavanagh
Joint Astronomy Centre, Hilo, Hawaii
2004 June
E-mail:ussc@star.rl.ac.uk
Copyright © 2004 Particle Physics and Astronomy Research Council